GPS carrier phase measurement representation and method of use

ABSTRACT

Sequential GPS Doppler carrier phase count measurements are used for precision sequential determination of position and velocity of a GPS receiver, such as for orbit determination and geolocation, with minimum throughput time. Real-time orbit determination and geolocation performance is enabled with an optimal sequential filter, and near-real-time performance is enabled with an optimal fixed-lag smoother. Many problems associated with prior art orbit determination are eliminated by addressing the “cycle slip” problem, the unknown initial range problem with RANGE CP  measurement representations, the problem of serial correlation in the measurements due to reprocessing of overlapping thermal noise. Also, the present invention significantly attenuates the carrier signal phase variation due to rotation of receiver antenna relative to transmitter antenna because the sequential phase count time intervals are sufficiently short.

BACKGROUND OF THE INVENTION

The GPS (Global Positioning System) consists, in part, of a constellation of NAVSTAR (Navigation System with Timing And Ranging) spacecraft with transmitters that continuously broadcast L-BAND radio carrier signals on two frequencies. NAVSTAR spacecraft all have near-circular orbits with radial distances that are 4.16 Earth radii from Earth center, with heights of 20182 km above the Earth's surface. With orbit period of 717.957 minutes and inclination to Earth's equator of 55 degrees, each NAVSTAR completes two orbits about the Earth in one sidereal day (a sidereal day is defined by one complete rotation of the Earth relative to the mean locations of a particular ensemble of stars, or to a particular ensemble of quasars. A solar day has 1440 minutes). NAVSTAR radio transmissions are directed towards the Earth.

USER spacecraft employ GPS receivers, and for most effective receipt of NAVSTAR radio transmissions, have orbits with radial distances that are significantly less than 4.16 Earth radii from Earth center. The large existing class of spacecraft in Low Earth Orbit (LEO) have radial distances that are in the neighborhood of 1.1 Earth radii from Earth center, with heights of roughly 600 km above the Earth's surface (a height of 637.81 km goes with radial distance of 1.1000 er). The orbits of USER spacecraft are estimated by processing measurements derived from NAVSTAR radio signals with the aid of GPS receivers. That is, GPS measurements are used for orbit determination of USER spacecraft equipped with GPS receivers.

Also, Earth-fixed GPS receivers are placed at unknown locations and are activated to collect GPS measurements. These are used to estimate the Earth-fixed receiver locations. We refer to this capability as geolocation.

There are two very different types of measurements derived from the NAVSTAR L-BAND radio carrier signals, namely: (i) pseudo-range measurements and (ii) Doppler carrier phase count measurements. Doppler carrier phase count measurements provide Doppler information on the relative velocity of USER spacecraft with respect to NAVSTAR spacecraft. This enables much more precise orbit estimates and geolocation estimates than those that process pseudo-range measurements only. The present invention refers to USER orbit determination and/or geolocation by processing Doppler carrier phase count measurements, not by processing pseudo-range measurements.

Measurement Representations

All methods of precise orbit determination and geolocation map measurement residuals linearly to state estimate corrections. A measurement residual is the difference between a measurement produced by receiver hardware and the estimated representation of the measurement derived from a state estimate—calculated on a computer. The measurement representation is critical to precise orbit determination and geolocation. In one aspect, the present invention refers most significantly to an improvement of the estimated representation of Doppler carrier phase count measurements.

Geodesy and Geophysics

Orbit determination of USER spacecraft, and geolocation of ground-fixed receivers, has been performed for several decades by processing GPS Doppler carrier phase count measurements. This has been particularly relevant for geodesy and geophysics, and very significant progress has been thereby achieved. But the measurement representations currently used in orbit determination and geolocation capabilities for geodesy and geophysics are fraught with serious problems, needlessly so. The Doppler carrier phase measurement is represented as a range measurement with unknown initial range. How can this be?

Every rigorous measurement representation equation for Doppler carrier phase is composed of several additive terms on the right, with the measurement representation on the left. Some terms on the right are characterized by signal, and some are characterized by noise. One of the terms for signal is called range-difference, or delta-range. This difference is: range at the end of the Doppler carrier phase count interval less range at the beginning of the Doppler carrier phase count interval, where range is a measure of distance between NAVSTAR transmitter and USER GPS receiver. One can rearrange the measurement representation equation so that the range-difference appears on the left, and is a function of the Doppler carrier phase measurement and other terms on the right. Algebraically one can then add the unknown range, at the beginning of the Doppler carrier phase count interval, to both sides of the equation. Now the sum of the unknown range on the left, at the beginning of the Doppler carrier phase count interval, and range-difference on the left defines the range at the end of the Doppler carrier phase count interval. That is, the modified equation presents the range at the end of the Doppler carrier phase count interval on the left as a function of the Doppler carrier phase measurement and the unknown range at the beginning of the Doppler carrier phase count interval, together with other terms, on the right. So orbit determination and geolocation for geodesy and geophysics treats the range at the end of the Doppler carrier phase count interval as the measurement, and requires an associated range measurement representation to form a measurement residual. This is how the Doppler carrier phase measurement is represented as a range measurement with unknown initial range. We shall call it the RANGE^(CP) measurement representation, with the superscript CP meaning that RANGE^(CP) is derived, in part, from a carrier phase measurement.

Further, the carrier phase measurements used for these range representations are overlapping measurements, not sequential measurements. This has a significant detrimental impact for orbit determination and geolocation, and is described below.

Presentation of Estimation Errors

The prior art geodesist presents small constant error magnitudes (i.e., those not derived directly from his state estimate error covariance matrix function) for his estimates of orbits and geolocations using overlapped RANGE^(CP) measurements, and has apparently convinced some technical people of their validity. These small error magnitudes usually refer to position components only, a limited subset of any complete state estimate. The argument has been made that if the geodesist is doing so well, then his estimation technique must surely be correct.

An extensive survey of the relevant literature has failed to identify a single analysis of the state estimate error, including a realistic error covariance. In fact, these analyses do not exist because of limitations in the prior art, including but not limited to the use of overlapped carrier phase measurements.

Each and every technique (including prior art methods of batch least squares, sequential filtering, batch filtering, and sequential smoothing) used by the geodesist to calculate precision estimates also calculates an associated state estimate error covariance matrix, or its inverse, that is used intrinsically to calculate the estimates. If these estimates are optimal and appropriately validated estimates, then their associated state estimate error covariance matrices are realistic. Realistic state estimate error covariance matrices would be invaluable for interpretation and use of orbit and geolocation estimates, but they are never presented. They are never presented because they are always significantly unrealistic. This is frequently admitted and is a problem with the prior art. Credible validation techniques in support of realistic state estimate error covariance presentations cannot be found. The present inventors have looked for them and have asked for them in appropriate places, but they apparently do not exist.

GPS Doppler Carrier Phase Count Measurements

NAVSTAR L-BAND radio carrier signals with specified frequencies are generated by atomic clocks on board each NAVSTAR. When received by any GPS receiver, the frequencies of these signals are Doppler shifted according to the deterministic theory of special and general relativity. The Doppler shift is proportional to the velocity of the USER receiver with respect to the velocity of the NAVSTAR transmitter. Each GPS receiver has its own local clock, and it is designed to create a radio signal with approximately the same frequency as that transmitted by each NAVSTAR. The incoming NAVSTAR Doppler shifted signal to each GPS receiver is differenced with the local receiver signal to isolate the Doppler shift and thereby generate a differenced Doppler phase with Doppler frequency. The Doppler phase is counted by the GPS receiver across a time interval [t_(m); t_(n)] defined by the receiver clock, where t_(m)<t_(n), and where m and n are time indices.

-   [00 sec, 10 sec], [10 sec; 20 sec], [20 sec; 30 sec], [30 sec; 40     sec], . . . sequential -   [00 sec, 10 sec], [00 sec; 20 sec], [00 sec; 30 sec], [00 sec; 40     sec], . . . overlapping

Define τ_(mn)=t_(n)−t_(m). Two illustrative sequences of four time intervals are displayed here, where the first sequence has a constant τ_(mn)=10 seconds (the constant sequential value for τ_(mn) will be orbit dependant and relatively small as compared to orbit period) and is sequential, but the second sequence is overlapped with non-constant τ_(mn) expanding without bound with each measurement. Each overlapped time interval is the concatenation of a sequence of adjacent sequential time intervals.

FIGS. 1A and 1B have general applicability and distinguish the sequential and overlapped Doppler measurement time intervals graphically.

The phase count measurement N_(mn) across each time interval [t_(m); t_(n) is the sum of an integer number of cycles plus a partial cycle. Thus the GPS Doppler carrier phase count measurement N_(mn) is a rational number (but typically not an integer), and has units of cycles. If the phase count time intervals are sequential, then the Doppler phase count measurements are sequential, non-overlapping, and τ_(mn) remains constant and small. But if the time intervals are overlapped, then the Doppler phase count measurements are overlapped, and τ_(mn) becomes indefinitely large. Each overlapped measurement is the sum of a sequence of adjacent sequential measurements.

Table 1 (sequential measurements) and Table 2 (overlapping measurements) present related examples (not that many other distinct and useful examples could be constructed and simplifications have been made for purposes of this example; ordinarily all calculations are performed in double precision to 15+decimals and time is represented in the Gregorian Calendar form or Julian Date) of simulated GPS Doppler carrier phase count measurement values for a GPS receiver on a spacecraft in LEO (Low Earth Orbit), referred to the same NAVSTAR transmitter. These tables are coordinated with the time intervals displayed above and with FIGS. 1A–1B. Columns 1, 2, 4, and 7 are the same for each table. Column 1 is time index, Column 2 is time t, Column 4 is range p, and Column 7 is the receiver phase count N_(0n) ^(R). Columns 3, 5, and 6 are different for each table due to the distinction in measurement time interval differences τ_(mn). Column 3 is time interval difference τ_(mn), Column 5 is delta-range Δp, and Column 6 is the measurement: N_(mn) for sequential measurement and N_(0n) for overlapping measurement.

TABLE 1 Sequential Doppler Carrier Phase Measurements τ_(mn) index t (sec) (sec) ρ (m) Δρ (m) N_(mn) (cy) N_(0n) ^(R) (cy) 0 00 18632055.19 0.00 10 −955.17 −5019.47 1 10 18631100.02 −5019.47 10 −274.49 −1442.44 2 20 18630825.53 −6461.91 10 406.08 2133.93 3 30 18631231.61 −4327.98 10 1086.39 5709.03 4 40 18632318.00 1381.05

The time-tag for each measurement is defined here to be the time at end of the Doppler count interval. Example for Table 1: For time interval [t_(m); t_(n)]=[20 seconds; 30 seconds], and sequential measurement N₂₃=2133.93 cycles, the time-tag t₃=30 seconds.

TABLE 2 Overlapped Doppler Carrier Phase Measurements τ_(mn) index t (sec) (sec) ρ (m) Δρ (m) N_(0n) (cy) N_(0n) ^(R) (cy) 0 00 18632055.19 0.00 10 −955.17 −5019.47 1 10 18631100.02 −5019.47 20 −1229.66 −6461.91 2 20 18630825.53 −6461.91 30 −823.58 −4327.98 3 30 18631231.61 −4327.98 40 262.81 1381.05 4 40 18632318.00 1381.05

BRIEF SUMMARY OF THE INVENTION

The present invention provides precision sequential orbit determination with minimum throughput time using sequential GPS Doppler carrier phase count measurements. Real-time orbit determination performance is enabled with an optimal sequential filter, and near-real-time performance is enabled with an optimal fixed-lag smoother. The present invention eliminates many problems associated with prior art orbit determination by addressing the “cycle slip” problem, the unknown initial range problem with RANGE^(CP) measurement representations, the problem of serial correlation in the measurements (due to reprocessing of overlapping thermal noise), and significantly attenuates the carrier signal phase variation (due to rotation of receiver antenna relative to transmitter antenna) because the sequential phase count time intervals are sufficiently short.

Construction of Sequential Doppler Phase Count Measurement Representations

Sequential Doppler phase count measurement representations are constructed:

-   1. to process sequential Doppler carrier phase count measurements     according to the new representation given by Eq. 10 (natural units:     cycles); -   2. to rigorously present each Doppler carrier phase count     measurement as a delta-range representation according to the new     expression defined by Eq. 21 (derived units: meters); -   3. to remove ionospheric effects with the two GPS L-BAND frequencies     according to Eq. 22; -   4. by choosing Eq. 6 rather than Eq. 8 for modeling USER clock     phenomenology; -   5. to remove USER spacecraft clock phenomenology with Doppler     measurement differences referred to distinct NAVSTARs according to     Eq. 30; -   6. to remove effects of USER spacecraft clock frequency steering,     when it exists, with Doppler measurement differences referred to     distinct NAVSTARs according to Eq. 30; and -   7. for processing in an optimal sequential filter, or optimal     sequential fixed-lag smoother, with autonomous measurement editor.

Considered individually, elements (1), (2), and (4) are new and unique. Considered individually, different versions of elements (3), (5), and (6) have been used in previous orbit determination capabilities. The optimal sequential filter referred to in element (7) has been produced by Analytical Graphics Inc., of Malvern Pa. (AGI), the assignees of the present invention, and is in current use by AGI customers.

The optimal fixed-lag smoother referred to in element (7) has been designed by AGI, but has not yet been implemented. Since the new element (1) is embedded in elements (3), (5), and (6), they are new in an embedded sense. Taken together, this combination of seven elements defines a new capability to perform precision sequential orbit determination with minimum throughput time using sequential GPS Doppler carrier phase count measurements. Real-time orbit determination performance is enabled with an optimal sequential filter, and near-real-time performance is enabled with an optimal fixed-lag smoother.

As mentioned above, the “cycle slip” problem is eliminated, the unknown initial range problem with RANGE^(CP) measurement representations is eliminated, serial correlation in the measurements (due to reprocessing of overlapping thermal noise) is eliminated, and the carrier signal phase variation (due to rotation of receiver antenna relative to transmitter antenna) is significantly attenuated because the sequential phase count time intervals are sufficiently short.

Elimination of the Cycle Slip Problem

The following example illustrates the cycle slip problem for overlapping measurements. Vast experience with overlapping measurements has shown the cycle slip problem to be a very significant problem in general. The present inventors submit, generally, that the processing of overlapping measurements is significantly inferior to the processing of sequential measurements by an optimal sequential filter.

EXAMPLE

From Table 1: At time-tag t=30 seconds, the sequential phase count measurement is N₂₃=2133.93 cycles, across time interval [20;30] seconds.

From Table 2: At time-tag t=30 seconds, the overlapping phase count measurement is N₀₃=−4327.98 cycles, across time interval [00;30] seconds.

Notice that: (−4327.98 cycles)=(−6461.91 cycles+2133.93 cycles), where (−4327.98 cycles) and (−6461.91 cycles) are overlapping measurements and (2133.93 cycles) is simultaneously a sequential measurement and a difference of overlapping measurements. These numbers represent valid measurements without cycle slip in this example; i.e., without loss of lock in the PLL (Phase Lock Loop).

Suppose now, as frequently happens with real data, that there is a loss of lock for sequential measurement N₂₃. That is, the receiver erroneously reports say N₂₃=10000.00 cycles, instead of the correct value N₂₃=2133.93 cycles for the sequential measurement. Then an erroneous overlapping measurement N₀₃ is reported as N₀₃=(−6461.91 cycles+10000.00 cycles)=(−3538.10 cycles), instead of the correct value N₀₃=(−4327.98 cycles).

Suppose further, as frequently happens, that the sequential measurement N₃₄=5709.03 cycles is reported correctly by the receiver. Then the overlapping incorrect measurement value N₀₄=(−3538.10 cycles+5709.03 cycles)=(2170.93 cycles) is reported by the receiver instead of the correct value of N₀₄=(1381.05 cycles). Sequential measurement N₃₄ is correct, but overlapping measurement N₀₄ is incorrect because overlapping measurement N₀₃ was incorrect.

Suppose further, as frequently happens, that sequential measurements N₄₅, N₅₆, N₆₇, . . . , following N₃₄ in this tracking pass, are reported correctly by the receiver. Then all overlapping measurements following N₀₄ will be reported incorrectly because they are additively chained to the incorrect overlapping measurement N₀₄. Overlapping measurements N₀₄, N₀₅, N₀₆, N₀₇, . . . are useless.

Overlapping Measurements

There are two cases to consider for the response of any estimator to the overlapping measurements. (i) If the estimator has an effective measurement editor, then overlapping measurements N₀₄, N₀₅, N₀₆, N₀₇, . . . will be appropriately discarded (note that this takes significant time in any operations) together with their associated measurement information, but (ii) If the estimator does not have an effective measurement editor, then some subset of the overlapping measurements N₀₄, N₀₅, N₀₆, N₀₇ . . . . will be accepted and processed for orbit determination. This will destroy the orbit estimate in the sense that the orbit estimate will incur very significant error.

In the first case the orbit estimate suffers a significant loss of information and is thereby degraded, and in the second case, the orbit estimate is destroyed. This is due to a cycle slip (loss of lock in the PLL) in a single sequential measurement N₂₃, and is referred to here as the cycle slip problem.

Sequential Measurements

Consider now the response of our optimal sequential filter to the sequential measurements: Erroneous measurement (N₂₃=10000.00 cycles) is rejected by the optimal sequential autonomous editor, but all other sequential measurements N₃₄, N₄₅, N₅₆, N₆₇ . . . . are accepted by the optimal sequential autonomous editor and appropriately used for sequential orbit determination. The only measurement information necessarily lost is that associated with measurement N₂₃. We refer to this as the elimination of the cycle slip problem.

The autonomous identification and rejection of any sequential carrier phase measurement that suffers loss of phase lock is accomplished in the following manner. Suppose a good sequential carrier phase measurement y_(k) at time t_(k) is used to correct the propagated a priori state estimate X_(k|k−1) at time t_(k) to calculate an improved state estimate X_(k|k) at time t_(k). Suppose the next measurement y_(k+1) at time t_(k+1) had a loss of phase lock, and is thus known to have a cycle slip. However, there is no way to determine that y_(k+1) is a bad cycle-slipped measurement by looking solely at the carrier phase measurement value. Rather the state estimate X_(k|k) and its realistic error covariance matrix P_(k|k) is propagated to time t_(k+1) to get X_(k+1|k) and P_(k+1|k,) and X_(k+1|k) is used to calculate a measurement representation y(X_(k+1|k)). The measurement residual Δy_(k+1)=y_(k+1)−y(X_(k+1|k)) is formed and the absolute value |Δy_(k+1) | is compared to a threshold T_(k+1) derived from P_(k+1|k) and from the measurement error variance matrix R_(k+1). If |Δy_(k+1)|<T_(k+1), then measurement y_(k+1) is accepted for processing by the optimal filter. But in the case of a cycle slip, we will find that |Δy_(k+1)|≧T_(k+1) and the measurement y_(k+1) is therefore autonomously rejected in real time.

Suppose the next sequential measurement y_(k+2) at time t_(k+2) is a good measurement (no cycle slip). Then we will find |Δy_(k+2)|<T_(k+2), and the measurement y_(k+2) is accepted for processing by the filter.

The autonomous real-time identification and rejection of cycle slips in sequential carrier phase measurements is enabled with the autonomous sequential editor, sequential estimator, and realistic covariance function.

This autonomous identification and rejection of flawed data is impossible with overlapped carrier phase measurements. A batch of overlapped carrier phase measurements are processed simultaneously with a batch estimator that prohibits autonomous editing, prohibits use of a realistic state error covariance function, and requires significant time to repair the damage done by a single sequential cycle slip.

Elimination of the Measurement Serial Correlation Problem

The processing of sequential measurements, in preference to overlapping measurements, eliminates the repeated exposure to the same thermal noise in the overlapping measurements that generates the serial correlation.

Elimination of the Unknown Initial Range Problem

Given only the GPS Doppler carrier phase count measurements N_(mn) and N_(0n) and their time-tags t_(n), all values of range ρ_(n) are unknown (the values of GPS pseudo-range have error magnitudes significantly larger than those of Δρ_(mn), derived from Doppler phase count). However, the range-difference Δρ_(mn), or delta-range, can be calculated from N_(mn) according to Eq. 21, and Δρ_(0n) can be calculated from N_(0n), also according to Eq. 21. From the definition of Δρ_(0n): Δρ_(0n)=ρ_(n)−ρ₀ That is: ρ_(n)=ρ₀+Δρ_(0n)  (1) for n ε {1, 2, . . . }. We shall refer to ρ₀ as the unknown initial range. Given the calculation of Δρ_(0n) from measurements N_(0n) for n ε {1, 2, . . . }, each unknown range ρ_(n) is treated by the geodesist as though it were a measurement, for n ε {1, 2, . . . }, with unknown initial range ρ₀. We refer to ρ_(n) above as ρ_(n)=RANGE^(CP).

The Unknown Initial Range Problem has three components: Communication, Estimation, and Throughput.

Communication

By definition, a measurement is a known value of an object or quantity determined by measuring it, but ρ_(n)=RANGE^(CP) is not measured and is not known. We have multiple contradictions (n ε {1, 2, . . . }) because the ρ_(n)=RANGE^(CP) are called measurements by the geodesist when they are not measurements. This is a problem in communication.

Estimation

From Eq. 1, we see that ρ₀ and Δρ_(0n) have distinct time-tags to and t_(n)>t₀. The unknown initial range ρ₀ is estimated, together with orbit parameters and other state parameters, from measurements N_(0n). But the execution of a state error transition function between times t₀ and t_(n) is required for each Δρ_(0n) to perform the estimation. The state error matrix includes errors on orbit parameters and errors on ρ₀. Significant cross correlations between orbit errors and errors on ρ₀ alias orbit errors and other state estimate errors into ρ₀ and thereby into ρ_(n) via Eq. 1. Conversely, errors on ρ₀ are aliased into orbit errors and other state estimate errors.

Orbit errors are due, in significant part, to force modeling errors. Thus ρ₀, ρ_(n), orbit errors, force modeling errors, and other state estimate errors are mutually contaminated. The geodesist wants to call ρ_(n)=RANGE^(CP) a measurement. Then his measurement modeling errors include orbit errors, force modeling errors, and other state estimate errors. This is a serious estimation problem where measurement errors are confused with, and not distinguished from, force modeling errors.

The estimation of ρ₀ must occur at its epoch to, but the geodesist prefers to ignore this fact and refers to ρ₀, implicitly and incorrectly, as a bias without epoch, to be estimated as an arbitrary constant. These estimation problems are serious.

Throughput

If one appropriately refers ρ₀ to its epoch to for estimation, then Δρ_(0n)=t_(n)−t₀ becomes large, and the propagation of state estimate and estimate error covariance matrix between times t₀ and t_(n) for each ρ_(n) consumes extremely excessive CPU time. This is a throughput problem that destroys, or degrades, any attempt to provide real-time state estimation.

Elimination

All three components of the Unknown Initial Range Problem are eliminated by processing sequential Doppler carrier phase count measurements N_(mn) with an optimal sequential filter, in preference to estimation of ρ₀ and calculation of ρ_(n) via Eq. 1 for use as pseudo-measurements.

BRIEF DESCRIPTION OF THE DRAWINGS

FIG. 1 illustrates graphically examples of sequential and overlapping time intervals for GPS Doppler phase count measurments;

FIG. 2 illustrates a flow chart of an embodiment of the process of the present invention.

FIG. 3 illustrates a flow chart for autonomous real-time identification and rejection of cycle slips in accordance with the present invention.

DETAILED DESCRIPTION OF THE INVENTION

One embodiment of the present invention

Sequential Doppler Phase Count Measurement Representations

The transmitter on each GPS spacecraft (NAVSTAR) emits radio carrier signals at two L-BAND frequencies f_(n) ^(NV) (NV indicates NAVSTAR and n is an integer denoting frequency, either 1 or 2). A USER spacecraft with GPS receiver detects radio carrier signals that are Doppler shifted with multiplicative Doppler shift β_(ij), and are contaminated by random additive ionospheric effects δf_(n) ^(ION). Thus the USER spacecraft receives radio carrier signals with frequency β_(ij)f_(n) ^(NV)+δf_(n) ^(ION). The USER receiver knows the nominal transmitted frequency {overscore (f)}_(n) ^(NV), and (using its own clock) approximates the received radio carrier signal with frequency f_(n) ^(U). A frequency difference is represented by the USER receiver to define (i.e., the subtraction order is defined by each actual receiver, and so our representation here may need a sign change for some receivers) the instantaneous Doppler frequency f_(n) ^(D): f _(n) ^(D) =f _(n) ^(U)−(β_(ij) f _(n) ^(NV) +δf _(n) ^(ION))  (2) with units cycles/second. Positive zero crossings (cycles) of f_(n) ^(D) are counted and summed (integrated) by the USER receiver, inclusive of a partial cycle, across a USER defined phase count interval Δt to construct a rational phase count number N_(j) ^(ni). Thus N_(j) ^(ni) consists of the sum of an integer number of cycles and a partial cycle. The GPS receiver phase lock loop incurs random thermal noise (Gaussian white noise) δN_(j) ^(ni), independent for each NAVSTAR link i, and independent at each measurement time-tag t_(j). Thus N_(j) ^(ni) has a representation with the sum (generalized integral):

$\begin{matrix} {N_{j}^{ni} = {{\int_{{t_{j}}^{{- \Delta}\; t}}^{t_{j}}{f_{n}^{D}{\mathbb{d}t}}} + {\delta\; N_{j}^{ni}}}} & (3) \end{matrix}$

The GPS sequential carrier phase measurement N_(j) ^(ni) is defined by Eqs. 2 and 3, and has units in cycles.

Thermal Noise Serial Correlation

It is important to notice that when sequential measurements are processed by any orbit determination algorithm, there is no serial correlation due to thermal noise δN_(j) ^(ni).

Random Clock Sampling Error

There exists a clock sampling error that generates a serial correlation coefficient value of 0.5 between each pair of sequential adjacent Doppler carrier phase count measurements. However, this correlation does not exist between measurements that are non-adjacent, and is therefore non-observable to the sequential estimator. Non-observable effects have no influence on the sequential estimator.

Calculation of Sequential Doppler Phase Count Measurement Representations

Referring now to Eq. 2, recall that NAVSTAR clock phenomenology is embedded in f_(n) ^(NV), and USER clock phenomenology is embedded in f_(n) ^(U). An explicit relation between f_(n) ^(U) and f_(n) ^(NV) is required, so define: δf _(n) ^(U) =f _(n) ^(U) −f _(n) ^(NV)  (4) We wish to embed δf_(n) ^(U) into Eq. 1 in order to identify δf_(n) ^(U) explicitly in the Doppler frequency f_(n) ^(D). From Eq. 4 we can write: f _(n) ^(U) =f _(n) ^(NV) +δf _(n) ^(U)  (5) and insert f_(n) ^(U) into Eq. 2 to get: f _(n) ^(D) =f _(n) ^(NV)(1−β_(ij))+δf _(n) ^(U) −δf _(n) ^(ION)  (6) or we can write: f _(n) ^(NV) =f _(n) ^(U) −δf _(n) ^(U)  (7) and insert f_(n) ^(NV) into Eq. 2 to get: f _(n) ^(D) =f _(n) ^(U)(1−β_(ij))+β_(ij) δf _(n) ^(U) −δf _(n) ^(ION)  (8)

The instantaneous Doppler frequency f_(n) ^(D) has different representations, that are defined by Eq. 6 and that are defined by Eq. 8. We shall return to this apparent ambiguity later.

Ionosphere

The ionospheric perturbation δf_(n) ^(ION) contained in the Doppler frequency f_(n) ^(D) has the representation:

$\begin{matrix} {{\delta\; f_{n}^{ION}} = {- {\left\lbrack {\frac{1.344536 \times 10^{- 7}}{f_{n}}\left( \frac{({Hz})({cycles})}{TECN} \right)} \right\rbrack\left\lbrack \frac{\mathbb{d}N_{TEC}}{\mathbb{d}t} \right\rbrack}}} & (9) \end{matrix}$ where the total electron content N_(TEC) is the integral of electron density along the path of the radio signal from transmitter to receiver, where f_(n) is evaluated in units Hz, dN_(TEC)/dt is evaluated in units TECN/s, and where1 TECN=1 electron/m². Then δf_(n) ^(ION) has units of Hz.

-   -   Sequential Doppler Carrier Phase Count Measurement         Representation for N_(j) ^(ni)

To find the representation for N_(j) ^(ni), insert Eq. 6 (this choice as opposed to Eq. 8 will be explained later) into Eq. 3 using Eq. 9: N _(j) ^(ni) ={overscore (f)} _(n) ^(NV)(ζ_(ij) +I _(j) ^(nNi))+{overscore (f)} _(n) ^(U) I _(j) ^(nU) +AΔN _(TEC) /└c{overscore (f)} _(n) ^(NV) ┘+δN _(j) ^(ni)  (10) where:

$\begin{matrix} {\zeta_{ij} = {{\int_{{t_{j}}^{{- \Delta}\; t}}^{t_{j}}{\left( {1 - \beta} \right){\mathbb{d}t}}} = {{\Delta_{\rho_{ij}}/c} - \chi_{ij}}}} & (11) \\ {\chi_{ij} = {\int_{{t_{j}}^{{- \Delta}\; t}}^{t_{j}}{\left\{ {{\frac{\mu}{c^{2}}\left\lbrack {\frac{1}{r_{j}} - \frac{1}{R_{i}}} \right\rbrack} + {\frac{1}{2c^{2}}\left\lbrack {{\overset{.}{s}}_{j}^{2} - {\overset{.}{S}}_{i}^{2}} \right\rbrack}} \right\}{\mathbb{d}t}}}} & (12) \\ {{\Delta\rho}_{ij} = {{\int_{{t_{j}}^{{- \Delta}\; t}}^{t_{j}}{{\overset{.}{\rho}}_{ij}{\mathbb{d}t}}} = {{\rho_{ij}\left( t_{j} \right)} - {\rho_{ij}\left( {t_{j} - {\Delta\; t}} \right)}}}} & (13) \end{matrix}$ ΔN _(TEC) =N _(TEC)(t _(j))−N _(TEC)(t _(j) −Δt)  (14) A=40.30816 (m³ Hz²/electron)  (15)

$\begin{matrix} {\beta_{ij} = {1 - {\frac{1}{c}{\overset{.}{\rho}}_{ij}} + {\frac{\mu}{c^{2}}\left\lbrack {\frac{1}{r_{j}} - \frac{1}{R_{i}}} \right\rbrack} + {\frac{1}{2c^{2}}\left\lbrack {{\overset{.}{s}}_{j}^{2} - {\overset{.}{S}}_{i}^{2}} \right\rbrack}}} & (16) \\ {I_{j}^{nNi} = {\int_{{t_{j}}^{{- \Delta}\; t}}^{t_{j}}{\left\lbrack \frac{\delta\; f_{n}^{N}}{{\overset{\_}{f}}_{n}^{N}} \right\rbrack\left( {1 - \beta_{ij}} \right){\mathbb{d}t}}}} & (17) \\ {I_{j}^{nU} = {\int_{{t_{j}}^{{- \Delta}\; t}}^{t_{j}}{\left\lbrack \frac{\delta\; f_{n}^{U}}{{\overset{\_}{f}}_{n}^{U}} \right\rbrack{\mathbb{d}t}}}} & (18) \end{matrix}$ where:

-   -   δN_(j) ^(ni) is receiver thermal noise, independent for each         NAVSTAR i     -   c is speed of light in a vacuum     -   μ is the geocentric two-body gravitational constant     -   r_(j) and {dot over (S)}_(i) are magnitudes of USER spacecraft         position and velocity vectors at time t_(j)     -   R_(i) and {dot over (S)}_(i) are magnitudes of NAVSTAR         spacecraft position and velocity vectors at time t_(i)     -   {dot over (ρ)}_(ij) is the range-rate ρ_(ij)=dp_(ij)/dt at time         t=t_(j)         -   ρ_(ij) is the range between NAVSTAR spacecraft at time t_(i)             and USER spacecraft at time t_(j)

In an alternate representation, Eq. 10 can also be written:

$\begin{matrix} {N_{j}^{ni} = {{\left( \frac{1}{\lambda_{n}} \right)\left\{ {{\Delta\;\rho_{ij}} - {c\;\chi_{ij}} + {c\left\lbrack {I_{j}^{nNi} + I_{j}^{nU}} \right\rbrack} + \left\lbrack \frac{A\;\Delta\; N_{TEC}}{\left( {\overset{\_}{f}}_{n}^{NV} \right)^{2}} \right\rbrack} \right\}} + {\delta\; N_{j}^{ni}}}} & (19) \end{matrix}$ where:

$\begin{matrix} {{{\lambda_{n}{\overset{\_}{f}}_{n}^{NV}} = c}{\lambda_{1} = {19.029367\frac{cm}{cycle}}}{\lambda_{2} = {24.42102\frac{cm}{cycle}}}} & (20) \end{matrix}$ Then solve Eq. 19 for Δρ_(ij) to write: Δρ_(ij)=λ_(n)(N _(j) ^(ni) −δN _(j) ^(ni))+c(x _(ij) [I _(j) ^(nNi) +I _(j) ^(nU)])−IAΔN_(TEC)/({overscore (f)} _(n) ^(NV)) ²  (21) Eq. 21 is useful for representation of Δρ_(ij) from that of N_(j) ^(ni). Two-Frequency Ionosphere Removal

For two-frequency ionosphere removal, let N_(j) ^(Ei) be defined by:

$\begin{matrix} {N_{j}^{Ei} = {\frac{{{\overset{\_}{f}}_{1}^{NV}N_{j}^{1i}} - {{\overset{\_}{f}}_{2}^{NV}N_{j}^{2i}}}{{\overset{\_}{f}}_{1}^{NV} - {\overset{\_}{f}}_{2}^{NV}} = \frac{{\gamma\; N_{j}^{1i}} - N_{j}^{2i}}{\gamma - 1}}} & (22) \end{matrix}$ where: y={overscore (f)} ₁ ^(NV) /{overscore (f)} ₂ ^(NV)  (23)

For orbit determination, use the representation {overscore (N)}_(j) ^(Ei);

$\begin{matrix} {{\overset{\_}{N}}_{j}^{Ei} = \frac{{{\overset{\_}{f}}_{1}^{NV}H_{j}^{1i}} - {{\overset{\_}{f}}_{2}^{NV}H_{j}^{2i}}}{{\overset{\_}{f}}_{1}^{NV} - {\overset{\_}{f}}_{2}^{NV}}} & (24) \end{matrix}$ where: H _(j) ^(ni) ={overscore (f)} _(n) ^(NV)ζ_(ij) +I _(j) ^(nNi) +I _(j) ^(nU) +δN _(j) ^(ni)  (25)

It is straightforward to demonstrate that ionospheric terms are eliminated due to use of Eqs. 22 and 24.

With respect to ionospheric wave length, Eq. 22 can be written:

$\begin{matrix} {N_{j}^{Ei} = \frac{{\lambda_{2}N_{j}^{1i}} - {\lambda_{1}N_{j}^{2i}}}{\lambda_{2} - \lambda_{1}}} & (26) \end{matrix}$ where λ_(n)f_(n)=c. Insert Eq. 19 into Eq. 26 and define: Δ{circumflex over (ρ)}_(ij) =E{Δρ _(ij) |N _(j) ^(ni)}  (27) Let λ_(ION) denote the two-frequency ionospheric wave length. Then: Δ{circumflex over (ρ)}_(ij)=λ_(ION) N _(j) ^(Ei) +cx _(ij) +E{I _(j) ^(Ni) |N _(j) ^(ni) }+E{I _(j) ^(U) |N _(j) ^(ni)}(28) where:

$\begin{matrix} {\lambda_{ION} = \frac{\lambda_{1}\lambda_{2}}{\lambda_{1} + \lambda_{2}}} & (29) \end{matrix}$ and where approximately λ_(ION)=10.69534 cm/cycle, given λ₁=19.029367 cm/cycle and λ₂=24.42102 cm/cycle.

First Differences on N_(j) ^(Ei)

With respect to first differences on N_(j) ^(Ei), we define: ΔN _(j) ^(E) =N _(j) ^(Ep) −N _(j) ^(Eq)  (30) where p and q refer to distinct NAVSTARS. Insert Eq. 22 into Eq. 30 to find that {overscore (f)}₁ ^(NV)I_(j) ^(1U) and {overscore (f)}₂ ^(NV) I_(j) ^(2U) are differenced out. That is, USER clock phase perturbations I_(j) ^(1U) and I_(j) ^(2U) vanish entirely due to first differences N_(j) ^(E) on ionosphere-free Doppler phase count measurements, and due to our choice of Eq. 6 rather than Eq. 8 for modeling USER clock phenomenology. NAVSTAR clock phase perturbations I_(j) ^(1Np), I_(j) ^(2Np), I_(j) ^(Nq), and I_(j) ^(2Nq) all survive, and all USER receiver PLL thermal noise perturbations δN_(j) ^(Ni) survive.

Serial Correlation Due to Overlapping Doppler Phase Count Measurements

With respect to overlapping carrier phase measurement, one can inspect Eq. 3 for time t_(j)=t₁ to write:

N₁^(ni) = ∫_(t_(j)^(−Δ t))^(t_(j))f_(n)^(D)𝕕t + δ N₁^(ni) and for time t_(j)=t₂ to write:

N₂^(ni) = ∫_(t₂^(−Δ t))^(t₂)f_(n)^(D)𝕕t + δ N₂^(ni) The overlapping measurement defined by the sum of the two sequential measurements can be represented with:

N₁^(ni) + N₂^(ni) = ∫_(t₂^(−2Δ t))^(t₂)f_(n)^(D)𝕕t + δ N_(1, 2)^(ni) where: δN _(1,2) ^(ni) =δN ₁ ^(ni) +δN ₂ ^(ni) The overlapping measurement defined by the sum of L sequential measurements can be defined with: N _(1,L) ^(ni) =N ₁ ^(ni) +N ₂ ^(ni) + . . . +N _(L) ^(ni);

By induction on the positive integers:

N_(1, L)^(ni) = ∫_(t₂^(−L Δ t))^(t₂)f_(n)^(D)𝕕t + δ N_(1, L)^(ni) where: δN _(1,L) ^(ni) =δN ₁ ^(ni) +δN ₂ ^(ni) + . . . +δN _(L) ^(ni)

Thermal Noise

It is important to notice that when overlapped Doppler phase count measurements N_(1,1) ^(ni), N_(1,2) ^(ni), . . . , N_(1,L) ^(ni) are processed by any orbit determination or geolocation capability, there is significant serial correlation in these measurements due to thermal noise component δN₁ ^(ni) in N_(1,1) ^(ni), N_(1,2) ^(ni), . . . , N_(1,L) ^(ni), also due to thermal noise component δN₂ ^(ni) in overlapped measurements N_(1,2) ^(ni), N_(1,3) ^(ni), . . . , N_(1,L) ^(ni), and, by induction on the positive integers, due to thermal noise component δN_(k) ^(ni) in overlapped measurements N_(1,k) ^(ni), N_(1,k+1) ^(ni), . . . , N_(1,L) ^(ni). The existence of the same thermal noise components in successive overlapped measurements generates serial correlations in the overlapped measurements. Optimal orbit determination requires that these serial correlations be explicitly accounted for when processing overlapped Doppler phase count measurements so that measurement residuals are properly mapped into state estimate corrections in the orbit determination and geolocation capabilities. However, these serial correlations are not accounted for by existing prior art capabilities that process overlapped Doppler phase count measurements.

Absence of Serial Correlation for Sequential Doppler Phase Count Measurements

There is no serial correlation in sequential Doppler phase count measurements due to thermal noise because thermal noise is Gaussian white noise, and white noise is independent with time. That is, white noise has no serial correlation with time.

A method for providing orbit determination and geolocation using sequential GPS Doppler phase count measurements has been described. It will be understood by those skilled in the art that the present invention may be embodied in other specific forms without departing from the scope of the invention disclosed and that the examples and embodiments described herein are in all respects illustrative and not restrictive. Those skilled in the art of the present invention will recognize that other embodiments using the concepts described herein are also possible. Further, any reference to claim elements in the singular, for example, using the articles “a,” “an,” or “the” is not to be construed as limiting the element to the singular. 

1. A method of refining state estimates of a Global Positioning System (GPS) receiver based upon sequential GPS carrier phase measurements, comprising: the GPS receiver periodically receiving, at a defined phase count interval Δt, Doppler-shifted carrier signals transmitted at two L-BAND frequencies f_(n) ^(NV) from a Navigation System with Timing And Ranging (NAVSTAR) spacecraft, where NV indicates NAVSTAR and n is an integer of either 1 or 2 denoting one of the L-BAND frequencies, and wherein the periodically received carrier signals are Doppler shifted with multiplicative Doppler shift β_(ij), for each NAVSTAR link i at a time-tag t_(j), and are contaminated by random additive ionospheric effects δf_(n) ^(ION) and wherein the GPS receiver approximates the nominal frequency {overscore (f)}_(n) ^(NV), at which the NAVSTAR spacecraft transmits, using the GPS receiver's internal clock; the GPS receiver approximating f_(n) ^(U) of the periodically received carrier signals using its internal clock; determining a frequency difference at the GPS receiver to define instantaneous Doppler frequency f_(n) ^(D) in units of cycles per second as: f _(n) ^(D) =f _(n) ^(NV)(1−β_(ij))+δf_(n) ^(U) −δf _(n) ^(ION); counting positive zero crossings of f_(n) ^(D), inclusive of a partial cycle, across the phase count interval Δt to measure a rational Doppler carrier phase count number N_(j) ^(ni) wherein N_(j)^(ni) = ∫_(t_(j)^(−Δ t))^(t_(j))f_(n)^(D)𝕕t + δ N_(j)^(ni) in units of cycles; calculating an estimated representation of Doppler carrier phase count number N_(j) ^(ni) using the formula: N _(j) ^(ni) ={overscore (f)} _(n) ^(NV)(ζ_(ij) +I _(j) ^(nNi))+{overscore (f)}_(n) ^(U) I _(j) ^(nU) +AΔN _(TEC) /└c{overscore (f)} _(n) ^(NV) ┘+δN _(j) ^(ni) where: ζ_(ij) = ∫_(j − Δ t)^(j)(1 − β)𝕕t  = Δ_(ρ ij)/c − ϰ_(ij) $ϰ_{ij} = {\int_{j - {\Delta\; t}}^{j}{\left\{ {{\frac{\mu}{c^{2}}\left\lbrack {\frac{1}{r_{j}} - \frac{1}{R_{i}}} \right\rbrack} + {\frac{1}{2c^{2}}\left\lbrack {{\overset{.}{s}}_{j}^{2} - {\overset{.}{S}}_{i}^{2}} \right\rbrack}} \right\}{\mathbb{d}t}}}$ ${\Delta\;\rho_{ij}} = {{\int_{j - {\Delta\; t}}^{j}{{\overset{.}{\rho}}_{ij}{\mathbb{d}t}}} = {{\rho_{ij}\left( t_{j} \right)} - {\rho_{ij}\left( {t_{j} - {\Delta\; t}} \right)}}}$ ΔN _(TEC) =N _(TEC)(t _(j))−N _(TEC)(t _(j) −Δt) A=40.30816 (m³Hz²/electron) $\beta_{ij} = {1 - {\frac{1}{c}{\overset{.}{\rho}}_{ij}} + {\frac{\mu}{c^{2}}\left\lbrack {\frac{1}{r_{j}} - \frac{1}{R_{i}}} \right\rbrack} + {\frac{1}{2c^{2}}\left\lbrack {{\overset{.}{s}}_{j}^{2} - {\overset{.}{S}}_{i}^{2}} \right\rbrack}}$ $I_{j}^{nNi} = {\int_{j - {\Delta\; t}}^{j}{\left\lbrack \frac{\delta\; f_{n}^{N}}{{\overset{\_}{f}}_{n}^{N}} \right\rbrack\left( {1 - \beta_{ij}} \right){\mathbb{d}t}}}$ $I_{j}^{nU} = {\int_{j - {\Delta t}}^{j}{\left\lbrack \frac{\delta\; f_{n}^{U}}{{\overset{\_}{f}}_{n}^{U}} \right\rbrack{\mathbb{d}t}}}$ where: δN_(j) ^(ni) is receiver thermal noise, independent for each NAVSTAR i, c is speed of light in a vacuum, μ is the geocentric two-body gravitational constant, r_(j) and {dot over (s)}_(j) are magnitudes of GPS receiver position and velocity vectors at time t_(j), R_(i) and {dot over (S)}_(i) are magnitudes of NAVSTAR spacecraft position and velocity vectors at time t_(i), {dot over (ρ)}_(ij) is the range-rate {dot over (ρ)}_(ij)=dp_(ij)/dt at time t=t_(j), ρ_(ij) is the range between NAVSTAR spacecraft at time t_(i) and GPS receiver at time t_(j), ζ_(ij) is a signal term with X_(ij) being a relativistic contribution, and I represent clock phase perturbations; differencing the measured and estimated representations of Doppler carrier phase count number N_(j) ^(ni) to obtain measurement residuals; mapping the measurement residuals to state estimate corrections; and applying the state estimate corrections to a priori state estimates.
 2. The method of claim 1, wherein the state estimates comprise a state estimate structure that contains GPS receiver position, GPS receiver velocity, and GPS receiver clock parameters.
 3. The method of claim 1, further comprising calculating each Doppler carrier phase count measurement as a delta-range (Δρ_(ij)) representation using: Δρ_(ij)=λ_(n)(N _(j) ^(ni) −δN _(j) ^(ni))+c(x _(ij) −[I _(j) ^(nNi) +I _(j) ^(nU)])−AΔN _(TEC)/({overscore (f)}_(n) ^(NV))².
 4. The method of claim 1, further comprising removing ionospheric effects by defining N_(j) ^(Ei) as: $N_{j}^{Ei} = {\frac{{{\overset{\_}{f}}_{1}^{NV}N_{j}^{1i}} - {{\overset{\_}{f}}_{2}^{NV}N_{j}^{2i}}}{{\overset{\_}{f}}_{1}^{NV} - {\overset{\_}{f}}_{2}^{NV}} = \frac{{\gamma\; N_{j}^{1i}} - N_{j}^{2i}}{\gamma - 1}}$ where γ={overscore (f)}₁ ^(NV)/{overscore (f)}₂ ^(NV).
 5. The method of claim 4, further comprising eliminating GPS receiver clock perturbations by taking a first difference of N_(j) ^(Ei) as ΔN_(j) ^(E)=N_(j) ^(Ep)−N_(j) ^(Eq) where p and q refer to distinct NAVSTARS.
 6. The method of claim 1, further comprising eliminating cycle slip by autonomous identification and rejection of any sequential carrier phase measurement that suffers loss of phase lock.
 7. The method of claim 6, further comprising continuing processing with a next acceptable sequential carrier phase measurement.
 8. The method of claim 7, wherein the autonomous identification and rejection of any sequential carrier phase measurement that suffers loss of phase lock further comprises: using sequential carrier phase measurement y_(k) at time t_(k) to correct a propagated a priori state estimate X_(k|k−1) at time t_(k) to calculate an improved state estimate X_(k|k) at time t_(k); propagating the state estimate X_(k|k) and its realistic error covariance matrix P_(k|k) to time t_(k+1) to get X_(k+1|k) and P_(k+1|k;) using X_(k+1|k) to calculate a measurement representation y(X_(k+t|k)); forming the measurement residual Δy_(k+1)=y_(k+1−y)(X_(k+1|k)); comparing the absolute value |Δy_(k+1) to a threshold T_(k+1) derived from P_(k+1|k) and from a measurement residual variance matrix R_(k+1,) such that: if |Δy_(k+1)|<T_(k+1,) then measurement y_(k+1) is accepted for processing; and if |Δy_(k+1) |≧T_(k+1,) the measurement y_(k+1) is autonomously rejected in real time.
 9. The method of claim 1, wherein serial correlation due to thermal noise δN_(j) ^(ni) in overlapping measurements is eliminated by processing sequential Doppler carrier phase count measurements.
 10. The method of claim 1, further comprising processing the state estimates in a sequential filter or a sequential smoother. 